HAL (France)open access
The magnetic and spin-down properties of slowly rotating fully convective M dwarfs
Stars low-mass, Stars rotation, 0, Stars magnetic fields
This document is indexed with metadata only — full text is not available in the archive for this record.
Open the official source ↗
Record · ID 354097
Retrieved via
Conceptio — every document is proof-bundled with source, license, and retrieval metadata.